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Tailored light-matter interaction through epsilon-near- zero modes

CLEO: QELS - Fundamental Science, CLEO_QELS 2015

Campione, Salvatore; Liu, Sheng L.; Benz, Alexander; Klem, John F.; Sinclair, Michael B.; Brener, Igal B.

We use epsilon-near-zero modes in semiconductor nanolayers to design a system whose spectral properties are controlled by their interaction with multi-dipole resonances. This design flexibility renders our platform attractive for efficient nonlinear composite materials. © OSA 2015.

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Nonpolar InGaN/GaN multi-quantum-well core-shell nanowire lasers

CLEO: Science and Innovations, CLEO-SI 2015

Li, Changyi; Wright, Jeremy B.; Liu, Sheng L.; Lu, Ping L.; Figiel, J.J.; Leung, Benjamin L.; Luk, Ting S.; Brener, Igal B.; Feezell, Daniel; Brueck, S.R.J.; Wang, George T.

Lasing is demonstrated from nonpolar III-nitride core-shell multi-quantum-well nanowires. The nanowire lasers were fabricated by coupling a top-down and bottom-up methodology and achieved lasing at wavelengths below the GaN bandedge. © OSA 2015.

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Control of strong light-matter coupling using the capacitance of metamaterial nanocavities

Nano Letters

Benz, Alexander; Campione, Salvatore; Klem, John F.; Sinclair, Michael B.; Brener, Igal B.

Metallic nanocavities with deep subwavelength mode volumes can lead to dramatic changes in the behavior of emitters placed in their vicinity. This collocation and interaction often leads to strong coupling. Here, we present for the first time experimental evidence that the Rabi splitting is directly proportional to the electrostatic capacitance associated with the metallic nanocavity. The system analyzed consists of different metamaterial geometries with the same resonance wavelength coupled to intersubband transitions in quantum wells.

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What is an epsilon-near-zero mode?

Integrated Photonics Research, Silicon and Nanophotonics, IPRSN 2015

Campione, Salvatore; Brener, Igal B.; Marquier, Francois

Metallic films much thinner than the skin depth can support surface plasmon modes whose dispersion approaches the plasma frequency, giving rise to the so-called epsilon-near-zero mode. We analyse its features and observation conditions. © 2015 OSA.

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Results 201–225 of 444
Results 201–225 of 444